Apollo-16 far-ultraviolet spectra in the Large Magellanic Cloud

1977 ◽  
Vol 211 ◽  
pp. 728 ◽  
Author(s):  
G. R. Carruthers ◽  
T. Page
2009 ◽  
Vol 703 (1) ◽  
pp. 736-751 ◽  
Author(s):  
Jorge L. Pineda ◽  
Jürgen Ott ◽  
Ulrich Klein ◽  
Tony Wong ◽  
Erik Muller ◽  
...  

2000 ◽  
Vol 538 (1) ◽  
pp. L61-L64 ◽  
Author(s):  
William P. Blair ◽  
Ravi Sankrit ◽  
Robin Shelton ◽  
Kenneth R. Sembach ◽  
H. Warren Moos ◽  
...  

1999 ◽  
Vol 117 (1) ◽  
pp. 206-224 ◽  
Author(s):  
Noah Brosch ◽  
Michael Shara ◽  
John MacKenty ◽  
David Zurek ◽  
Brian McLean

1997 ◽  
Vol 114 ◽  
pp. 1945 ◽  
Author(s):  
Andrew A. Cole ◽  
Jeremy R. Mould ◽  
John S., III Gallagher ◽  
John T. Clarke ◽  
John T. Trauger ◽  
...  

2013 ◽  
Vol 9 (S296) ◽  
pp. 388-389
Author(s):  
Ananta C. Pradhan ◽  
Amit Pathak ◽  
Jayant Murthy ◽  
D. K. Ojha

AbstractWe have presented the observations of O VI absorption at 1032 Å towards 22 sightlines in 10 superbubbles (SBs) of the Large Magellanic Cloud (LMC) using the data obtained from the Far Ultraviolet Spectroscopic Explorer (FUSE). The estimated abundance of O VI in the SBs varies from a minimum of (1.09 ±0.22)×1014 atoms/cm2 in SB N206 to a maximum of (3.71±0.23)×1014 atoms/cm2 in SB N70. We find about a 46% excess in the abundance of O VI in the SBs compared to the non-SB lines of sight. Even inside a SB, O VI column density (N(O VI)) varies by about a factor of 2 to 2.5. These data are useful in understanding the nature of the hot gas in SBs.


2010 ◽  
Vol 718 (2) ◽  
pp. L141-L144 ◽  
Author(s):  
Ananta C. Pradhan ◽  
Amit Pathak ◽  
Jayant Murthy

2007 ◽  
Vol 664 (1) ◽  
pp. 304-321 ◽  
Author(s):  
Parviz Ghavamian ◽  
William P. Blair ◽  
Ravi Sankrit ◽  
John C. Raymond ◽  
John P. Hughes

2000 ◽  
Vol 538 (1) ◽  
pp. L39-L42 ◽  
Author(s):  
S. D. Friedman ◽  
J. C. Howk ◽  
B-G Andersson ◽  
K. R. Sembach ◽  
T. B. Ake ◽  
...  

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